MERLIN outstations are not available since April 2011 until further notice.

The phased-array WSRT is no longer vailable, only a single dish.

***NEW***:
The following telescopes have been upgraded to 2 Gbit/s: Ef, Hh, Mc, Nt, On, Ys.
Still limited to 1 Gbit/s: Tr, Wb1, Jb, Sh, Mh.
Arecibo is limited to 512 Mbit/s without UT restriction (as from October 2013),
up to 72 hours per month. Mixed-bandwidth observations are possible.

The current limitation for real-time e-VLBI correlation is estimated to be
8 telescopes at 2 Gbit/s, or 15 telescopes at 1 Gbit/s. For example, 6 stations
at 2 Gbit/s + 3 stations at 1 Gbit/s, or 5 stations at 2 Gbit/s and 4 stations
at 1 Gbit/s should be possible.

Scheduled e-EVN runs

16 January 2018, 13:00 UTC

20:44 GST

17 January 2018, 13:00 UTC

20:48 GST

* 4 February 2018, 13:00 UTC

5 February 2018, 13:00 UTC

6 February 2018, 13:00 UTC

22:06 GST

7 February 2018, 13:00 UTC

22:10 GST

27 March 2018, 13:00 UTC

1:20 GST

28 March 2018, 13:00 UTC

1:24 GST

10 April 2018, 13:00 UTC

2:15 GST

11 April 2018, 13:00 UTC

2:19 GST

17 May 2018, 13:00 UTC

4:41 GST

18 May 2018, 13:00 UTC

4:45 GST

19 June 2018, 13:00 UTC

6:51 GST

20 June 2018, 13:00 UTC

6:55 GST

18 September 2018, 13:00 UTC

12:50 GST

19 September 2018, 13:00 UTC

12:54 GST

16 October 2018, 13:00 UTC

14:40 GST

17 October 2018, 13:00 UTC

14:44 GST

20 November 2018, 13:00 UTC

16:58 GST

21 November 2018, 13:00 UTC

17:02 GST

4 December 2018, 13:00 UTC

17:53 GST

5 December 2018, 13:00 UTC

17:57 GST

The observing frequency in a session is decided based on proposal pressure